{"as_of":"2026-08-18T00:20:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:40badb15dc1a0a33fa6efdc6ee4084074e9d93882980dca04bbfac9e01c7fea8","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T14:56:30.727147Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-14T22:13:04.293474Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1809.09845","last_updated":"2019-07-12T08:06:22Z","snapshot_observed_at":"2026-08-14T18:23:26.603483Z","submitted_at":"2018-09-26T08:27:34Z","title":"Assessing the effect of lens mass model in cosmological application with updated galaxy-scale strong gravitational lensing sample","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.09845","snapshot_observed_at":"2026-08-07T14:56:30.727147Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.17262","last_updated":"2025-05-22T20:16:33Z","snapshot_observed_at":"2026-08-15T05:39:24.357094Z","submitted_at":"2025-05-22T20:16:33Z","title":"A Joint Analysis of Strong Lensing and Type Ia Supernovae to Determine the Hubble Constant","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-07T14:56:30.727147Z"},"links":{"cited_paper":"/paper/1809.09845","citing_paper":"/paper/2505.17262"},"observation_digest":"sha256:556baff2c62b3b47af3bb5157ddce4ab4885575e2cefabcedb00b96c21974a18","observation_id":"394ea8ef-6fb2-40bb-9086-ee8fcd70233f","resolution":{"observed_at":"2026-08-07T14:56:30.727147Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.09845","last_updated":"2019-07-12T08:06:22Z","snapshot_observed_at":"2026-08-14T18:23:26.603483Z","submitted_at":"2018-09-26T08:27:34Z","title":"Assessing the effect of lens mass model in cosmological application with updated galaxy-scale strong gravitational lensing sample","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.09845","snapshot_observed_at":"2026-08-04T00:32:26.977062Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:26.977062Z"},"links":{"cited_paper":"/paper/1809.09845","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:bf3d2ec90b6f55d5b8d3bd35d36fa9a1513cd945f748edf8c1d0f79d557d09c6","observation_id":"ddb3a9a1-7488-4f12-b479-9077071e6840","resolution":{"observed_at":"2026-08-04T00:32:26.977062Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.09845","last_updated":"2019-07-12T08:06:22Z","snapshot_observed_at":"2026-08-14T18:23:26.603483Z","submitted_at":"2018-09-26T08:27:34Z","title":"Assessing the effect of lens mass model in cosmological application with updated galaxy-scale strong gravitational lensing sample","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.09845","snapshot_observed_at":"2026-07-13T21:03:53.845854Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2603.21127","last_updated":"2026-03-22T08:51:18Z","snapshot_observed_at":"2026-08-14T16:50:54.144766Z","submitted_at":"2026-03-22T08:51:18Z","title":"Testing General Relativity on Galactic Scales via DESI-BAO and Strong Lensing: Circumventing Assumptions on the Hubble Constant, Sound Horizon, and Dark Energy","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-07-13T21:03:53.845854Z"},"links":{"cited_paper":"/paper/1809.09845","citing_paper":"/paper/2603.21127"},"observation_digest":"sha256:e0c59a1f989c689898c25f34798c244ec942f50dba533d8d7ae68fe66fd122dd","observation_id":"08ed3bdc-0fec-45a7-bdd1-797592c92c64","resolution":{"observed_at":"2026-07-13T21:03:53.845854Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.09845","last_updated":"2019-07-12T08:06:22Z","snapshot_observed_at":"2026-08-14T18:23:26.603483Z","submitted_at":"2018-09-26T08:27:34Z","title":"Assessing the effect of lens mass model in cosmological application with updated galaxy-scale strong gravitational lensing sample","version":5},"cited_work":{"arxiv_id":"1809.09845","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1809.09845","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"ec8655ad-bd46-4830-ba54-f79a81aca75c","year":2019},"citing_paper":{"arxiv_id":"2603.27616","last_updated":"2026-04-09T07:03:12Z","snapshot_observed_at":"2026-08-17T17:22:48.696974Z","submitted_at":"2026-03-29T10:21:42Z","title":"Model-independent test of the cosmic distance duality relation with recent observational data","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-05-14T22:11:51.900263Z"},"links":{"cited_paper":"/paper/1809.09845","citing_paper":"/paper/2603.27616"},"observation_digest":"sha256:67ee3b4c22f36762c5396181f12e674102a79d16cb8712e500ed9a9bc1220d25","observation_id":"ceece148-f6e2-49e1-974b-12575734c7e0","resolution":{"observed_at":"2026-05-14T22:13:04.298044Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1809.09845/citation-record","integrity":"/paper/1809.09845/integrity","json":"/paper/1809.09845/citation-record.json","paper":"/paper/1809.09845"},"outbound":[],"paper":{"arxiv_id":"1809.09845","last_updated":"2019-07-12T08:06:22Z","latest_version":5,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-14T18:23:26.603483Z","submitted_at":"2018-09-26T08:27:34Z","title":"Assessing the effect of lens mass model in cosmological application with updated galaxy-scale strong gravitational lensing sample"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1809.09845."}